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Coherent network analysis technique for discriminating gravitational-wave bursts from instrumental noise

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dc.contributor.authorChatterji, Shourov
dc.contributor.authorLazzarini, A
dc.contributor.authorStein, Leo
dc.contributor.authorSutton, Patrick
dc.contributor.authorSearle, Antony
dc.contributor.authorTinto, M
dc.date.accessioned2015-12-07T22:22:44Z
dc.date.issued2006
dc.date.updated2015-12-07T09:08:27Z
dc.description.abstractThe sensitivity of current searches for gravitational-wave bursts is limited by non-Gaussian, nonstationary noise transients which are common in real detectors. Existing techniques for detecting gravitational-wave bursts assume the output of the detector
dc.identifier.issn0556-2821
dc.identifier.urihttp://hdl.handle.net/1885/20364
dc.publisherAmerican Physical Society
dc.sourcePhysical Review D
dc.titleCoherent network analysis technique for discriminating gravitational-wave bursts from instrumental noise
dc.typeJournal article
local.bibliographicCitation.lastpage18
local.bibliographicCitation.startpage082005/1
local.contributor.affiliationChatterji, Shourov, California Institute of Technology
local.contributor.affiliationLazzarini, A, California Institute of Technology
local.contributor.affiliationStein, Leo, California Institute of Technology
local.contributor.affiliationSutton, Patrick, California Institute of Technology
local.contributor.affiliationSearle, Antony, College of Physical and Mathematical Sciences, ANU
local.contributor.affiliationTinto, M, California Institute of Technology
local.contributor.authoruidSearle, Antony, u9719170
local.description.notesImported from ARIES
local.identifier.absfor010504 - Mathematical Aspects of General Relativity
local.identifier.ariespublicationu4103646xPUB12
local.identifier.citationvolume74
local.identifier.doi10.1103/PhysRevD.74.082005
local.identifier.scopusID2-s2.0-33749853916
local.type.statusPublished Version

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